The comparison of the KOM using the NEA reference model with the known NEA population from the MPC for objects with H _V ≤ 23 mag (the proxy of objects larger than ∼140 m). The orbital elements of perihelion distance, eccentricity, and inclination are shown from left to right. The KOM applied to 10 random realizations of the NEA reference model is shown in gray, while the MPC distribution is shown in blue.